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Galactic and Cosmic Chemical Evolution with Hypernovae

Chiaki Kobayashi
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Abstract

We provide new nucleosynthesis yields depending on metallicity and energy (i.e., (normal supernovae and hypernovae), and show the evolution of heavy element abundances from C to Zn in the solar neighborhood. We then show the chemodynamical simulation of the Milky Way Galaxy and discuss the G-dwarf problem. We finally show the cosmological simulation and discuss the galaxy formation and chemical enrichment.

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Chiaki Kobayashi. 2005-08-09. Galactic and Cosmic Chemical Evolution with Hypernovae. https://doi.org/10.1017/s1743921305005880

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